Bose-Einstein Condensate Dark Matter Halos Confronted with Galactic Rotation Curves

<div>Best fit curves for the HSB II. galaxy sample. The solid black lines hold for the baryonic matter + BEC model, while the dashed red lines hold for the baryonic matter + NFW model. The BEC model does not describe well the extended flat regions.</div>

Advances in High Energy Physics

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Figure 2

Figure 2: Bose-Einstein Condensate Dark Matter Halos Confronted with Galactic Rotation Curves 